sunspots – regions of strong magnetic activity. sunspots are cooler than the rest of the...
TRANSCRIPT
![Page 1: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/1.jpg)
SUN - VOCABULARY
![Page 2: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/2.jpg)
Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem to move across the Sun as the Sun rotates. The number of sunspots changes over time. They follow a cycle, peaking in number every 11 years. An average sunspot is about the size of Earth.
![Page 3: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/3.jpg)
•Prominence – clouds of gas that make loops and jets that extend into the corona from the photosphere. They sometimes last for weeks.
![Page 4: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/4.jpg)
Flares – sudden increases in brightness that often occur near sunspots or prominences. They are violent eruptions that last from minutes to hours.
![Page 5: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/5.jpg)
Suns Layers Corona – suns outermost
atmosphere Chromosphere – thin layer
below Corona Photosphere – 1st visible part
of sun Convective region – area
where gasses circulate Radiative zone – thickest
layer Core – suns energy produced
by nuclear fusion
![Page 6: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/6.jpg)
Shadows
Umbra The central,
darker part of the shadow where light is totally blocked.
Penumbra The lighter
part of the shadow where light is partially blocked.
![Page 7: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/7.jpg)
Solar Eclipse – When the moons shadow appears on Earth.
The moon is between the Earth and the Sun.
Can be partial or total – depends on whether you are in the path of the Umbra or the Penumbra.
Total eclipses only occur when you are in the Umbra.
![Page 8: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/8.jpg)
Lunar Eclipse – Occurs when the Moon moves into the Earth’s shadow.
Earth is between the Sun and the Moon.
A lunar Eclipse can occur only during a full Moon.
Unlike solar eclipses – lunar eclipses can be seen from anywhere on Earth where it’s nighttime.
![Page 9: Sunspots – regions of strong magnetic activity. Sunspots are cooler than the rest of the photosphere and appear as dark splotches on the Sun. They seem](https://reader035.vdocument.in/reader035/viewer/2022072006/56649f445503460f94c647a6/html5/thumbnails/9.jpg)
Tides